The Vimos VLT Deep Survey. Stellar mass segregation and large-scale galaxy environment in the redshift range 0.2 < z < 1.4
- Scodeggio, Marco
- Vergani, D.
- Cucciati, O.
- Iovino, Angela
- Franzetti, P.
- Garilli, Bianca
- Lamareille, Fabrice
- Bolzonella, M.
- Pozzetti, L.
- Abbas, U.
- Marinoni, Christian
- Contini, Thierry
- Bottini, D.
- Le Brun, V.
- Le Fèvre, Olivier
- Maccagni, D.
- Scaramella, R.
- Tresse, Laurence
- Vettolani, G.
- Zanichelli, A.
- Adami, C.
- Arnouts, S.
- Bardelli, Sandro
- Cappi, A.
- Charlot, Stéphane
- Ciliegi, Paolo
- Foucaud, S.
- Gavignaud, I.
- Guzzo, L.
- Ilbert, Olivier
- Mccracken, Henry J.
- Marano, B.
- Mazure, A.
- Meneux, Baptiste
- Merighi, R.
- Paltani, S.
- Pello, R.
- Pollo, Agnieszka
- Radovich, M.
- Zamorani, G.
- Zucca, E.
- Bondi, M.
- Bongiorno, Angela
- Brinchmann, J.
- de la Torre, Sylvain
- de Ravel, L.
- Gregorini, L.
- Memeo, P.
- Pérez-Montero, E.
- Mellier, Yannick
- Temporin, Sonia
- Walcher, C. Jakob
DOIAbstract
International audienceContext: Hierarchical models of galaxy formation predict that the properties of a dark matter halo depend on the large-scale environment surrounding the halo. As a result of this correlation, we expect massive haloes to be present in larger number in overdense regions than in underdense ones. Given that a correlation exists between a galaxy stellar mass and the hosting dark matter halo mass, the segregation in dark matter halo mass should then result in a segregation in the distribution of stellar mass in the galaxy population. Aims: In this work we study the distribution of galaxy stellar mass and rest-frame optical color as a function of the large-scale galaxy distribution using the VLT VIMOS Deep Survey sample, in o...
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